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Fig. C.3.

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Posteriors of the hyperparameters related to the variation in α in redshift are shown. The dark blue dashed lines in the one-dimensional distributions represent the priors. The hyperparameters shown here are the (ascending) power-law index αz of the modeled merger rate, and then hyperparameters connected to varying α from Eq. (2). This includes αlow, αhigh, the width of the sigmoid log(Δzα) and the middle of the sigmoid z ¯ α $ \bar z_{\alpha } $. We also plot the difference between the high-redshift and low-redshift value Δα, which now is a Gaussian, because the difference of two Gaussians is once again a Gaussian distribution variable.

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